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For other uses, see Light year (disambiguation).
As defined by the International Astronomical Union (IAU), a light-year ( or light year) is the distance that light travels in a vacuum in one Julian year.[1] The speed of light is 299,792,458 metres per second. Therefore, a light-year (symbol: ly) is a unit of length, equal to just under 1013 kilometres. The light-year is often used to measure distances to stars and other distances on a galactic scale, especially in non-specialist and popular science publications. The preferred unit in astrometry is the parsec, because it can be more easily derived from, and compared with, observational data. The parsec is defined as the distance at which an object will appear to move one arcsecond of parallax when the observer moves one astronomical unit perpendicular to the line of sight to the observer, and is equal to approximately 3.26 light-years.[1] The related unit of the light-month, roughly one-twelfth of a light-year, is also used occasionally for approximate measures.[2][3]
[edit] Numerical value
A light-year is equal to:
The figures above are based on a Julian year (not Gregorian year) of exactly 365.25 days (each of exactly 86,400 SI seconds, totalling 31,557,600 seconds)[4] and a defined speed of light of 299,792,458 m/s, both included in the IAU (1976) System of Astronomical Constants, used since 1984.[5] The DE405 value of the astronomical unit, 149,597,870,691 m,[6] is used for the light-year in astronomical units and parsecs. The light-month does not have a precise definition or value, as there is no unique definition of a month in astronomical or SI units: however it may be understood to be approximately one-twelfth of a light-year, in line with the various mundane definitions of the month (hollow month, average Julian month, etc.). [edit] Other valuesBefore 1984, the tropical year (not the Julian year) and a measured (not defined) speed of light were included in the IAU (1964) System of Astronomical Constants, used from 1968 to 1983.[7] The product of Simon Newcomb's J1900.0 mean tropical year of 31,556,925.9747 ephemeris seconds and a speed of light of 299,792.5 km/s produced a light-year of 9.460530 × 1015 metres (rounded to the seven significant digits in the speed of light) found in several modern sources[8][9][10] was probably derived from an old source such as a reputable 1973 reference[11] which was not updated until 2000.[12] Other high precision values are not derived from a coherent IAU system. A value of 9.460536207 × 1015 metres found in some modern sources[13][14] is the product of a mean Gregorian year of 365.2425 days (31,556,952 s) and the defined speed of light (299,792,458 m/s). The Live Search value, 9.460528405 × 1015 metres,[15] is the product of the J1900.0 mean tropical year and the defined speed of light. [edit] Distances in light-yearsDistances measured in fractions of a light-year (or in light-months) usually involve objects within a star system. Distances measured in light-years include distances between nearby stars, such as those in the same spiral arm or globular cluster. One kilolight-year, abbreviated "kly", is one thousand light-years, or about 307 parsecs. Kilolight-years are typically used to measure distances between parts of a galaxy. One megalight-year, abbreviated "Mly", is one million light-years, or about 306,600 parsecs. Megalight-years are typically used to measure distances between neighboring galaxies and galaxy clusters. One gigalight-year, abbreviation "Gly", is one billion light-years—one of the largest distance measures used. One gigalight-year is about 306.6 million parsecs. Gigalight-years are typically used to measure distances to supergalactic structures, including quasars and the Great Wall.
[edit] See alsoThis audio file was created from a revision dated 27 June 2005, and does not reflect subsequent edits to the article. (Audio help)
[edit] References
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